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A&A 463, L5-L8 (2007)
DOI: 10.1051/0004-6361:20066568
Letter
XMM-Newton observations of PSR B1957+20
H. H. Huang and W. BeckerMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, 85748 Garching, Germany
e-mail: rhuang@mpe.mpg.de
(Received 13 October 2006 / Accepted 9 January 2007)
Abstract
We report on XMM-Newton observations of the "Black Widow pulsar", PSR B1957+20.
The pulsar's X-ray emission is non-thermal and best modeled with a single powerlaw spectrum
of photon index
2.03+0.51-0.36. No coherent X-ray pulsations at the pulsar's
spin-period could be detected, though a strong binary-phase dependence of the X-ray flux
is observed for the first time. The data suggest that the majority of the pulsar's X-radiation
is emitted from a small part of the binary orbit only. We identified this part as being near
to where the radio eclipse takes place. This could mean that the X-rays from PSR B1957+20 are
mostly due to intra-shock emission which is strongest when the pulsar wind interacts with the
ablated material from the companion star.
Key words: pulsars: individual: PSR B1957+20 -- stars: neutron -- X-rays: stars -- binaries: eclipsing
© ESO 2007
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